Astronomy:(523684) 2014 CQ23

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Short description: Trans-Neptunian object in the classical Kuiper belt


(523684) 2014 CQ23
Discovery[1]
Discovered byPan-STARRS 1
Discovery siteHaleakalā Obs.
Discovery date13 March 2011
Designations
(523684) 2014 CQ23
2014 CQ23
Minor planet categoryTNO[2] · cubewano[3]
p-DP[4] · distant[1]
Orbital characteristics[2]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter· 1[1]
Observation arc16.04 yr (5,857 d)
|{{{apsis}}}|helion}}53.658 AU
|{{{apsis}}}|helion}}38.670 AU
46.164 AU
Eccentricity0.1623
Orbital period313.66 yr (114,565 d)
Mean anomaly302.71°
Mean motion0° 0m 11.16s / day
Inclination8.6867°
Longitude of ascending node30.646°
236.86°
Physical characteristics
Mean diameter321 km (est.)[3]
343 km (est.)[4]
Geometric albedo0.08 (assumed)[4]
0.09 (assumed)[3]
Absolute magnitude (H)5.7[1][2]


(523684) 2014 CQ23 (provisional designation 2014 CQ23) is a trans-Neptunian object and cubewano from the Kuiper belt, located in the outermost region of the Solar System. It was discovered on 13 March 2011, by astronomers with the Pan-STARRS survey at Haleakala Observatory, Hawaii, United States.[1] The classical Kuiper belt object belongs to the hot population and is a dwarf planet candidate, as it measures approximately 330 kilometers (210 miles) in diameter.

Orbit and classification

2014 CQ23 is a cubewano, a classical, low-eccentricity object in the Kuiper belt, located in between the two resonant plutino and twotino populations, and belongs to the "stirred" hot population rather than to the cold population with low inclinations.

It orbits the Sun at a distance of 38.7–53.7 AU once every 313 years and 8 months (114,565 days; semi-major axis of 46.16 AU). Its orbit has an eccentricity of 0.16 and an inclination of 9° with respect to the ecliptic.[2]

Numbering and naming

This minor planet was numbered by the Minor Planet Center on 25 September 2018 and received the number 523687 in the minor planet catalog (M.P.C. 111779).[5] As of 2018, it has not been named.[1]

Physical characteristics

According to the American astronomer Michael Brown, 2014 CQ23 measures 343 kilometers in diameter based on an assumed albedo of 0.08.[4] On his website, Michael Brown lists this object as a "possible" dwarf planet (200–400 km), which is the category with the lowest certainty in his 5-class taxonomic system.[4] Similarly, Johnston's archive estimates a diameter 321 kilometers using an albedo of 0.09.[3] As of 2018, neither a spectral type or the color indices have been determined, nor a rotational lightcurve has been obtained from spectroscopic and photometric observations. The body's color, rotation period, pole and shape remain unknown.[2][6]

References

External links